Free Access

Fig. C.1.


Top panel: stellar mass distribution for sample collected in this work. Blue- and red-shaded histograms refer to the samples of SFGs (i.e. MS and SMGs) and dusty AGN. Bottom panel: specific star formation rate sSFR/sSFRMS distributions for the same samples in the top panel. The sSFRMS is derived according to the relation of Speagle et al. (2014). In the figure, we also show the separation between normal MS galaxies and SBs at log(sSFR/sSFRMS)=0.6.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.